Zobrazeno 1 - 10
of 123 932
pro vyhledávání: '"Energy transport"'
Autor:
Chen, Ziming1,2,3 (AUTHOR), Zhou, Tianjun2,3 (AUTHOR) zhoutj@lasg.iap.ac.cn, Chen, Xiaolong2 (AUTHOR), Zhang, Lixia2 (AUTHOR), Qian, Yun1 (AUTHOR), Wang, Zeyi2,3,4 (AUTHOR), He, Linqiang2,3 (AUTHOR), Leung, L. Ruby1 (AUTHOR)
Publikováno v:
Journal of Climate. Sep2024, Vol. 37 Issue 18, p4647-4666. 20p.
Autor:
Cherubini, Anna Maria, Gidea, Marian
We describe a mechanism for transport of energy in a mechanical system consisting of a pendulum and a rotator subject to a random perturbation. The perturbation that we consider is the product of a Hamiltonian vector field and a scalar, continuous, s
Externí odkaz:
http://arxiv.org/abs/2409.03132
Autor:
Opsahl, Catherine D., Jiang, Yuan, Grubb, Samantha A., Okinaka, Alan T., Chlanda, Nicolaus A., Conley, Hannah S., Kirk, Aidan T., Spielman, Sarah E., Carroll, Thomas J., Noel, Michael W.
A static electric field of a few V/cm shifts the energy levels of ultracold Rydberg atoms in a magneto-optical trap. For a given principle quantum number, most of the energy levels are nearly degenerate at zero field and fan out with increasing field
Externí odkaz:
http://arxiv.org/abs/2407.21764
Recent studies have shown that vertical enthalpy transport can explain the inflated radii of highly irradiated gaseous exoplanets. They have also shown that rotation can influence this transport, leading to highly irradiated, rapidly rotating, object
Externí odkaz:
http://arxiv.org/abs/2407.15602
Autor:
Nawagamuwage, Sithara U., Williams, Elliot S., Islam, Md Muhaiminul, Parshin, Igor V., Burin, Alexander L., Busschaert, Nathalie, Rubtsov, Igor V.
In an effort to increase the speed and efficiency of ballistic energy transport via oligomeric chains, we performed measurements of the transport in compounds featuring long alkyl chains of up to 37 methylene units. Compounds of the N3-(CH2)n-COOMe t
Externí odkaz:
http://arxiv.org/abs/2405.13776
Recent JWST eclipse spectra of the high-density hot Saturn HD 149026b between 2.35 and 5.08 $\mu$m has allowed for in-depth study of its atmosphere. To understand its atmospheric properties, we have created a grid of 1D radiative-convective-thermoche
Externí odkaz:
http://arxiv.org/abs/2404.17658